Andronov, Ivan L.Antoniuk, K. A.Baklanov, A. V.Breus, V. V.Burwitz, V.Chinarova, L. L.Chochol, D.Dubovsky, P. A.Han, W.Hegedus, T.Henden, A.Hric, L.Kim, Chun-HweyKim, YonggiKolesnikov, S. V.Kudzej, I.Liakos, A.Niarchos, P. G.Oksanen, A.Patkos, L.Petrik, K.Pit, N. V.Shakhovskoy, N. M.Virnina, N. A.Yoon, J.Zola, S.2014-03-132014-03-132010-07Odessa Astronomical Publicationshttps://dspace.onu.edu.ua/handle/123456789/4586Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 07/2010 . – Vol.23.We present a review of highlights of our photometric and photo-polarimetric monitoring and mathematical modeling of interacting binary stars of di erent types classical, asynchronous, intermediate polars with 25 timescales corresponding to di erent physical mechanisms and their combinations (part "Polar"); negative and positive superhumpers in nova-like and dwarf novae stars ("Superhumper"); symbiotic ("Symbiosis"); eclipsing variables with and without evidence for a current mass transfer ("Eclipser") with a special emphasis on systems with a direct impact of the stream into the gainor star's atmosphere, which we propose to call "Impactors", or V361 Lyr-type stars. Other parts of the ILA project are "Stellar Bell" (pulsating variables of di erent types and periods - M, SR, RV Tau, RR Lyr, Delta Sct) and "New Variable"enVariable starscataclysmicpulsatingeclipsinginteracting binaryArticle